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Projekt Druckansicht

Untersuchungen der Kompakte Sterne mit schweren Baryonen und Quarks: zweite Periode

Fachliche Zuordnung Kern- und Elementarteilchenphysik, Quantenmechanik, Relativitätstheorie, Felder
Astrophysik und Astronomie
Förderung Förderung von 2020 bis 2024
Projektkennung Deutsche Forschungsgemeinschaft (DFG) - Projektnummer 433859871
 
Erstellungsjahr 2025

Zusammenfassung der Projektergebnisse

This project continued into the second stage the exploration of compact stars with a focus on their properties related to the behavior of high-density matter that contains heavy baryons (hyperons and ∆-resonances) and quarks. The key idea was to extend the existing codes for heavy-baryon and quark matters and computation of key thermodynamic quantities of such matter, including equation of state and composition at non-zero temperature. These results were compared to the macroscopic properties of compact stars, such as mass, radius, moment of inertia, and deformability to place constraints on the underlying models. We have also continued the studies of transport properties of dense matter, in particular, the bulk viscosity of nucleonic matter. The focus has been on the muon component in the matter in neutrino transparent and trapped regimes. As a first application of the obtained finitetemperature equations of state of hyperonic matter, we have computed static and rapidly rotating hot compact star configurations. Our nucleonic and hyperonic equations of state were exported to the CompOSE repository for the use of the numerical relativity community.

Link zum Abschlussbericht

https://doi.org/10.34657/23838

Projektbezogene Publikationen (Auswahl)

 
 

Zusatzinformationen

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